Milne-Eddington inversion of the Fe I line pair at 630 nm: (Research note)

Astronomy and Astrophysics

Volumn 518, Issue 9, 2010, Pages

  Orozco Suarez D ^a   Bellot Rubio, L R ^b   Del Toro Iniesta, J C ^b  

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^b INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

Author keywords

Line: profiles; Methods: data analysis; Polarization; Radiative transfer; Sun: photosphere; Sun: surface magnetism

Indexed keywords

DATA REDUCTION; MAGNETIC FIELDS; OPACITY; POLARIZATION; RADIATIVE TRANSFER; THERMODYNAMICS;

CONSTANT RATIO; EDDINGTON APPROXIMATIONS; LINE INVERSIONS; LINE: PROFILES; MAGNETOHYDRODYNAMIC SIMULATIONS; METHODS:DATA ANALYSIS; OPACITY RATIO; PHYSICAL CONDITIONS; QUIET SUN; SOLAR PHOTOSPHERE; SUN: PHOTOSPHERE; THERMODYNAMIC PARAMETER; TWO-LINE; VECTOR MAGNETIC FIELDS;

SUN;

EID: 77955781502     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014374     Document Type: Article

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